Regression of non-linear coupling of noise in LIGO detectors. (1st February 2018)

• Record Type: Journal Article
• Authors: Da Silva Costa, C F; Billman, C; Effler, A; Klimenko, S; Cheng, H-P
• Is Part Of: Classical and quantum gravity. Volume 35:Number 5(2018:Mar.)
• Publication Date: 2018-02-01
• Subjects: gravitational waves -- instrumental noise -- noise regression; Quantum gravity -- Periodicals; Gravitation -- Periodicals; Relativity (Physics) -- Periodicals; Space and time -- Periodicals; Periodicals; 521.1
• DOI: 10.1088/1361-6382/aaa536
• Languages: English
• ISSNs: 0264-9381

Abstract

Abstract: In 2015, after their upgrade, the advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors started acquiring data. The effort to improve their sensitivity has never stopped since then. The goal to achieve design sensitivity is challenging. Environmental and instrumental noise couple to the detector output with different, linear and non-linear, coupling mechanisms. The noise regression method we use is based on the Wiener–Kolmogorov filter, which uses witness channels to make noise predictions. We present here how this method helped to determine complex non-linear noise couplings in the output mode cleaner and in the mirror suspension system of the LIGO detector.